Kohno calculated the \(g\)  matrix for the symmetric nuclear matter,
using the Brueckner-Hartree-Fock method with chiral N\(^{3}\) LO 2NFs and NNLO 3NFs [1]}.
He set \(c_D=-2.5\)  and \(c_E=0.25\)  so that the energy per nucleon can become minimum
at \(\rho = \rho _{0}\) .
Toyokawa et al. localized the non-local chiral \(g\)  matrix into three-range Gaussian forms [2]}, using the localization method proposed
by the Melbourne group [3]}, [4]}, [5]}.
The resulting local \(g\)  matrix is referred to as “Kyushu \(g\) -matrix”.
